! Started logfile: /scr/pima/bg219b_uvs/J0920-3631_S_dfm.log on Thu May 19 20:11:14 2016 float field_size field_size = 1024 float field_cell field_cell = 0.5000 float taper_size taper_size = 20.0 float freq freq = 2.22000 obs /scr/pima/bg219b_uvs/J0920-3631_S_uva.fits ! Reading UV FITS file: /scr/pima/bg219b_uvs/J0920-3631_S_uva.fits ! AN table 1: 24 integrations on 28 of 28 possible baselines. ! AN table 2: 24 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.939732 visibilities/baseline/integration-bin. ! Found source: J0920-3631 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 2.22e+09 3.2e+07 1 3.2e+07 ! 02 2 2.252e+09 3.2e+07 1 3.2e+07 ! 03 3 2.284e+09 3.2e+07 1 3.2e+07 ! 04 4 2.348e+09 3.2e+07 1 3.2e+07 ! ! Polarization(s): RR ! ! Read 54 lines of history. ! ! Reading 5052 visibilities. select rr, 1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16 ! Restricting channel ranges to the available 4 channels. ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 print "field_size =", field_size ! field_size = 1024 print "field_cell =", field_cell ! field_cell = 0.5 print "taper_size =", taper_size ! taper_size = 20 ![@/opt64/bin/pima_mupet_01.dfm J0920-3631_S] float lim_self lim_self = 120.0 float lim_val lim_va = 1.2 integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 1024x1024 pixels with 0.500x0.500 milli-arcsec cellsize. startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.014534Jy sigma=14.984106 ! Fit after self-cal, rms=0.844710Jy sigma=12.268136 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.097 mas, bmaj=15.03 mas, bpa=13.94 degrees ! Estimated noise=1.03791 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.116355 Jy ! Component: 100 - total flux cleaned = 0.156321 Jy ! Total flux subtracted in 100 components = 0.156321 Jy ! Clean residual min=-0.011477 max=0.020292 Jy/beam ! Clean residual mean=-0.000204 rms=0.003963 Jy/beam ! Combined flux in latest and established models = 0.156321 Jy ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 37 components and 0.156321 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.110089Jy sigma=1.528303 ! Fit after self-cal, rms=0.109760Jy sigma=1.525325 ! Inverting map print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.915 mas, bmaj=16.76 mas, bpa=13.44 degrees ! Estimated noise=0.697449 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0336012 Jy ! Component: 100 - total flux cleaned = 0.0505782 Jy ! Component: 150 - total flux cleaned = 0.059745 Jy ! Component: 200 - total flux cleaned = 0.0650497 Jy ! Total flux subtracted in 200 components = 0.0650497 Jy ! Clean residual min=-0.008356 max=0.009858 Jy/beam ! Clean residual mean=-0.000071 rms=0.002836 Jy/beam ! Combined flux in latest and established models = 0.22137 Jy ! Performing phase self-cal ! Adding 79 model components to the UV plane model. ! The established model now contains 107 components and 0.22137 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100714Jy sigma=1.355033 ! Fit after self-cal, rms=0.100583Jy sigma=1.353526 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.915 x 16.76 at 13.44 degrees (North through East) ! Clean map min=-0.0083044 max=0.14329 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! NL 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! NL 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! NL 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! NL 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! FD 0.96 HN 1.11 KP 0.86 LA 0.90 ! NL 1.08 OV 0.93 PT 1.18 SC 1.02 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! NL 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! FD 0.92 HN 1.14 KP 0.94 LA 0.88 ! NL 1.02 OV 0.99 PT 1.14 SC 0.94 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! NL 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! ! Fit before self-cal, rms=0.100583Jy sigma=1.353526 ! Fit after self-cal, rms=0.100776Jy sigma=1.343611 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.916 mas, bmaj=16.89 mas, bpa=13.48 degrees ! Estimated noise=0.693491 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00125565 Jy ! Component: 100 - total flux cleaned = 0.00160644 Jy ! Component: 150 - total flux cleaned = 0.00184838 Jy ! Component: 200 - total flux cleaned = 0.00196079 Jy ! Total flux subtracted in 200 components = 0.00196079 Jy ! Clean residual min=-0.007158 max=0.008814 Jy/beam ! Clean residual mean=-0.000035 rms=0.002542 Jy/beam ! Combined flux in latest and established models = 0.223331 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 122 components and 0.223331 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100683Jy sigma=1.342534 ! Fit after self-cal, rms=0.100711Jy sigma=1.342269 ! Inverting map selfcal true, true, soltime1 ! Performing amp+phase self-cal over 120 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100711Jy sigma=1.342269 ! Fit after self-cal, rms=0.100561Jy sigma=1.342248 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=3.913 mas, bmaj=16.88 mas, bpa=13.47 degrees ! Estimated noise=0.693268 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000242875 Jy ! Component: 100 - total flux cleaned = 0.000405732 Jy ! Component: 150 - total flux cleaned = 0.00045722 Jy ! Component: 200 - total flux cleaned = 0.000504603 Jy ! Total flux subtracted in 200 components = 0.000504603 Jy ! Clean residual min=-0.007215 max=0.008798 Jy/beam ! Clean residual mean=-0.000034 rms=0.002533 Jy/beam ! Combined flux in latest and established models = 0.223836 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 130 components and 0.223836 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100504Jy sigma=1.341627 ! Fit after self-cal, rms=0.100496Jy sigma=1.341593 flux_cutoff = imstat(rms) * dynam ! Inverting map repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -1.98059e-05 Jy ! Component: 100 - total flux cleaned = 7.40773e-05 Jy ! Component: 150 - total flux cleaned = 0.000159692 Jy ! Component: 200 - total flux cleaned = 0.000201345 Jy ! Total flux subtracted in 200 components = 0.000201345 Jy ! Clean residual min=-0.007206 max=0.008772 Jy/beam ! Clean residual mean=-0.000034 rms=0.002525 Jy/beam ! Combined flux in latest and established models = 0.224037 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 135 components and 0.224037 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100454Jy sigma=1.341124 ! Fit after self-cal, rms=0.100453Jy sigma=1.341098 ! Inverting map selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100453Jy sigma=1.341098 ! Fit after self-cal, rms=0.100338Jy sigma=1.341087 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=3.911 mas, bmaj=16.87 mas, bpa=13.46 degrees ! Estimated noise=0.692967 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 4.44237e-05 Jy ! Component: 100 - total flux cleaned = 0.000128855 Jy ! Component: 150 - total flux cleaned = 0.000207618 Jy ! Component: 200 - total flux cleaned = 0.000246148 Jy ! Total flux subtracted in 200 components = 0.000246148 Jy ! Clean residual min=-0.007233 max=0.008732 Jy/beam ! Clean residual mean=-0.000033 rms=0.002517 Jy/beam ! Combined flux in latest and established models = 0.224283 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 140 components and 0.224283 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100304Jy sigma=1.340699 ! Fit after self-cal, rms=0.100303Jy sigma=1.340674 flux_cutoff = imstat(rms) * dynam ! Inverting map repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -5.76876e-05 Jy ! Component: 100 - total flux cleaned = 1.59411e-05 Jy ! Component: 150 - total flux cleaned = 5.0794e-05 Jy ! Component: 200 - total flux cleaned = 8.55073e-05 Jy ! Total flux subtracted in 200 components = 8.55073e-05 Jy ! Clean residual min=-0.007241 max=0.008715 Jy/beam ! Clean residual mean=-0.000033 rms=0.002512 Jy/beam ! Combined flux in latest and established models = 0.224369 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 144 components and 0.224369 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100275Jy sigma=1.340361 ! Fit after self-cal, rms=0.100275Jy sigma=1.340337 ! Inverting map uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths. win_mult = win_mult * 1.2 selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100275Jy sigma=1.340337 ! Fit after self-cal, rms=0.100274Jy sigma=1.340330 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=8.706 mas, bmaj=29.36 mas, bpa=1.175 degrees ! Estimated noise=0.778229 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00114445 Jy ! Component: 100 - total flux cleaned = 0.00108836 Jy ! Component: 150 - total flux cleaned = 0.0010344 Jy ! Component: 200 - total flux cleaned = 0.00108374 Jy ! Total flux subtracted in 200 components = 0.00108374 Jy ! Clean residual min=-0.008813 max=0.011256 Jy/beam ! Clean residual mean=-0.000042 rms=0.003513 Jy/beam ! Combined flux in latest and established models = 0.225453 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 151 components and 0.225453 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100285Jy sigma=1.340189 ! Fit after self-cal, rms=0.100251Jy sigma=1.339984 flux_cutoff = imstat(rms) * dynam ! Inverting map repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000100286 Jy ! Component: 100 - total flux cleaned = -8.17248e-06 Jy ! Component: 150 - total flux cleaned = -1.14459e-05 Jy ! Component: 200 - total flux cleaned = -1.55076e-05 Jy ! Total flux subtracted in 200 components = -1.55076e-05 Jy ! Clean residual min=-0.008804 max=0.011211 Jy/beam ! Clean residual mean=-0.000042 rms=0.003501 Jy/beam ! Combined flux in latest and established models = 0.225437 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 152 components and 0.225437 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100274Jy sigma=1.340037 ! Fit after self-cal, rms=0.100236Jy sigma=1.339884 ! Inverting map uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Estimated beam: bmin=3.91 mas, bmaj=16.87 mas, bpa=13.46 degrees ! Estimated noise=0.693057 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.91 x 16.87 at 13.46 degrees (North through East) ! Clean map min=-0.0070543 max=0.14319 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=3.087 mas, bmaj=15.16 mas, bpa=13.96 degrees ! Estimated noise=1.03104 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.115257 Jy ! Component: 100 - total flux cleaned = 0.156313 Jy ! Component: 150 - total flux cleaned = 0.180086 Jy ! Component: 200 - total flux cleaned = 0.195052 Jy ! Total flux subtracted in 200 components = 0.195052 Jy ! Clean residual min=-0.009315 max=0.010713 Jy/beam ! Clean residual mean=-0.000104 rms=0.002689 Jy/beam ! Combined flux in latest and established models = 0.195052 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 59 model components to the UV plane model. ! The established model now contains 59 components and 0.195052 Jy ! Inverting map and beam ! Estimated beam: bmin=3.91 mas, bmaj=16.87 mas, bpa=13.46 degrees ! Estimated noise=0.693057 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0139201 Jy ! Component: 100 - total flux cleaned = 0.0211103 Jy ! Component: 150 - total flux cleaned = 0.0252773 Jy ! Component: 200 - total flux cleaned = 0.0267122 Jy ! Total flux subtracted in 200 components = 0.0267122 Jy ! Clean residual min=-0.007351 max=0.008936 Jy/beam ! Clean residual mean=-0.000037 rms=0.002557 Jy/beam ! Combined flux in latest and established models = 0.221764 Jy ! Adding 66 model components to the UV plane model. ! The established model now contains 113 components and 0.221764 Jy ! Inverting map uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=8.706 mas, bmaj=29.36 mas, bpa=1.175 degrees ! Estimated noise=0.778229 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00239137 Jy ! Component: 100 - total flux cleaned = 0.00274728 Jy ! Component: 150 - total flux cleaned = 0.00298897 Jy ! Component: 200 - total flux cleaned = 0.00327087 Jy ! Total flux subtracted in 200 components = 0.00327087 Jy ! Clean residual min=-0.008593 max=0.011531 Jy/beam ! Clean residual mean=-0.000041 rms=0.003543 Jy/beam ! Combined flux in latest and established models = 0.225035 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000130038 Jy ! Component: 100 - total flux cleaned = 0.000192887 Jy ! Component: 150 - total flux cleaned = 0.000250858 Jy ! Component: 200 - total flux cleaned = 0.000306608 Jy ! Total flux subtracted in 200 components = 0.000306608 Jy ! Clean residual min=-0.008633 max=0.011512 Jy/beam ! Clean residual mean=-0.000040 rms=0.003528 Jy/beam ! Combined flux in latest and established models = 0.225342 Jy ! Adding 34 model components to the UV plane model. ! The established model now contains 137 components and 0.225342 Jy ! Inverting map uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=3.91 mas, bmaj=16.87 mas, bpa=13.46 degrees ! Estimated noise=0.693057 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000500667 Jy ! Component: 100 - total flux cleaned = -0.000619715 Jy ! Component: 150 - total flux cleaned = -0.000667556 Jy ! Component: 200 - total flux cleaned = -0.00062144 Jy ! Total flux subtracted in 200 components = -0.00062144 Jy ! Clean residual min=-0.007134 max=0.008626 Jy/beam ! Clean residual mean=-0.000031 rms=0.002514 Jy/beam ! Combined flux in latest and established models = 0.22472 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 159 components and 0.22472 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100310Jy sigma=1.340545 ! Fit after self-cal, rms=0.100282Jy sigma=1.340448 wmodel /J0920-3631_S_map.mod ! wmodel: Unable to open new model file: /J0920-3631_S_map.mod ! Error occured in command: wmodel ![Exited script file: /opt64/bin/pima_mupet_01.dfm] ! wmap /scr/pima/bg219b_uvs/J0920-3631_S_map.fits ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.91 x 16.87 at 13.46 degrees (North through East) ! Clean map min=-0.0069927 max=0.14155 Jy/beam ! Writing clean map to FITS file: /scr/pima/bg219b_uvs/J0920-3631_S_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.14155 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00251153 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -5.32292 5.32292 10.6458 21.2917 42.5833 85.1667 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0075 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.141 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 56.36 quit ! Quitting program ! Log file /scr/pima/bg219b_uvs/J0920-3631_S_dfm.log closed on Thu May 19 20:11:17 2016